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1952 Hesburgh

From Wikipedia, the free encyclopedia
Main-belt asteroid

1952 Hesburgh
Discovery[1]
Discovered byIndiana University
(Indiana Asteroid Program)
Discovery siteGoethe Link Obs.
Discovery date3 May 1951
Designations
(1952) Hesburgh
Named after
Theodore M. Hesburgh
(University president)[2]
1951 JC · 1936 ND
1939 AB · 1940 GQ
1954 XC · 1974 KQ
main-belt · (outer)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc77.14 yr (28,177 days)
Aphelion3.5522AU
Perihelion2.6708 AU
3.1115 AU
Eccentricity0.1416
5.49yr (2,005 days)
175.77°
0° 10m 46.56s / day
Inclination14.255°
78.149°
339.27°
Physical characteristics
Dimensions32.39±8.33 km[4]
35.55±1.4 km(IRAS:15)[5]
37.501±0.151 km[6]
39.660±0.381 km[7]
41.27±1.19 km[8]
47.7±0.1h[9][a]
0.078±0.005[8]
0.080±0.012[6]
0.0837±0.0130[7]
0.10±0.03[4]
0.1041±0.009(IRAS:15)[5]
Tholen = CD:[1] · CD:[3]
B–V = 0.756[1]
U–B = 0.340[1]
10.31±0.33[10] · 10.32[1][3][5][8][7][4]

1952 Hesburgh, provisional designation1951 JC, is a rare-type carbonaceousasteroid from the outer regions of theasteroid belt, approximately 37 kilometers in diameter.

It was discovered on 3 May 1951, byIU'sIndiana Asteroid Program atGoethe Link Observatory near Brooklyn, Indiana, United States.[11] It was named for FatherTheodore M. Hesburgh.[2]

Orbit and classification

[edit]

Hesburgh orbits the Sun in theouter main-belt at a distance of 2.7–3.6 AU once every 5 years and 6 months (2,005 days). Its orbit has aneccentricity of 0.14 and aninclination of 14° with respect to theecliptic.[1] It was first identified as1936 ND atJohannesburg Observatory in 1936. The body'sobservation arc begins at Goethe, five days after its official discovery observation.[11]

Physical characteristics

[edit]

Lightcurve

[edit]

In March 2005, a rotationallightcurve ofHesburgh was obtained from photometric observations by American astronomerBrian Warner at his Palmer Divide Observatory in Colorado. Lightcurve analysis gave a longer-than averagerotation period of 47.7 hours with a brightness variation of at least 0.18magnitude (U=2).[9][a]

Spectral type

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In theTholen taxonomy,Hesburgh is a rare CD:spectral type,[1] an intermediary between the common carbonaceousC-type asteroid and the darkD-type asteroid, which is typical among theJupiter trojans beyond the main-belt. Another asteroid with a CD:-type is691 Lehigh.

Diameter and albedo

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According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite, and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Hesburgh measures between 32.39 and 41.27 kilometers in diameter and its surface has analbedo between 0.078 and 0.1041.[4][5][6][7][8] TheCollaborative Asteroid Lightcurve Link adopts the results obtained by IRAS, that is, an albedo of 0.1041 and a diameter of 35.55 kilometers with anabsolute magnitude of 10.32.[3]

Naming

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Thisminor planet was named after AmericanTheodore M. Hesburgh (1917–2015), a priest and president of theUniversity of Notre Dame in Notre Dame, Indiana. He was also a member of theNational Science Board and played a decisive role for the founding of theKitt Peak National Observatory, as well as of the ChileanCerro Tololo Interamerican Observatory during the 1960s.[2] The approved naming citation was published by theMinor Planet Center on 1 January 1981 (M.P.C. 5688).[12]

Notes

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  1. ^abLightcurve plot of (1952) Hesburgh, Palmer Divide Observatory,B. D. Warner (2005). Due to a period of nearly 2 days, the photometric observations were more or less in sync with the body's rotation and no lightcurve maxima could be covered by either of the two consecutive observation sessions. The lightcurve amplitude could be larger than 0.18 magnitude.

References

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  1. ^abcdefgh"JPL Small-Body Database Browser: 1952 Hesburgh (1951 JC)" (2017-06-02 last obs.).Jet Propulsion Laboratory. Retrieved2 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1952) Hesburgh".Dictionary of Minor Planet Names – (1952) Hesburgh.Springer Berlin Heidelberg. p. 157.doi:10.1007/978-3-540-29925-7_1953.ISBN 978-3-540-00238-3.
  3. ^abcd"LCDB Data for (1952) Hesburgh". Asteroid Lightcurve Database (LCDB). Retrieved5 April 2017.
  4. ^abcdNugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015)."NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos".The Astrophysical Journal.814 (2): 13.arXiv:1509.02522.Bibcode:2015ApJ...814..117N.doi:10.1088/0004-637X/814/2/117. Retrieved5 April 2017.
  5. ^abcdTedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004)."IRAS Minor Planet Survey V6.0".NASA Planetary Data System.12: IRAS-A-FPA-3-RDR-IMPS-V6.0.Bibcode:2004PDSS...12.....T. Retrieved22 October 2019.
  6. ^abcMasiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014)."Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos".The Astrophysical Journal.791 (2): 11.arXiv:1406.6645.Bibcode:2014ApJ...791..121M.doi:10.1088/0004-637X/791/2/121. Retrieved5 April 2017.
  7. ^abcdMainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results".The Astrophysical Journal.741 (2): 25.arXiv:1109.6407.Bibcode:2011ApJ...741...90M.doi:10.1088/0004-637X/741/2/90.
  8. ^abcdUsui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011)."Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey".Publications of the Astronomical Society of Japan.63 (5):1117–1138.Bibcode:2011PASJ...63.1117U.doi:10.1093/pasj/63.5.1117. (online,AcuA catalog p. 153)
  9. ^abWarner, Brian D. (December 2005)."Asteroid lightcurve analysis at the Palmer Divide Observatory – spring 2005".The Minor Planet Bulletin.32 (4):90–92.Bibcode:2005MPBu...32...90W.ISSN 1052-8091. Retrieved5 April 2017.
  10. ^Veres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015)."Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 – Preliminary results".Icarus.261:34–47.arXiv:1506.00762.Bibcode:2015Icar..261...34V.doi:10.1016/j.icarus.2015.08.007. Retrieved5 April 2017.
  11. ^ab"1952 Hesburgh (1951 JC)".Minor Planet Center. Retrieved5 April 2017.
  12. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved5 April 2017.

External links

[edit]
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